HFI energetic particle effects: characterization, removal, and simulation

Research output: Contribution to journalJournal article – Annual report year: 2015Researchpeer-review

Standard

HFI energetic particle effects: characterization, removal, and simulation. / Ade, P. A. R.; Aghanim, N.; Armitage-Caplan, C.; Arnaud, M.; Ashdown, M.; Atrio-Barandela, F.; Aumont, J.; Baccigalupi, C.; Banday, A. J.; Barreiro, R. B.; Battaner, E.; Benabed, K.; Benoit, A.; Benoit-Levy, A.; Bernard, J. -P.; Bersanelli, M.; Bielewicz, P.; Bobin, J.; Bock, J. J.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Bridges, M.; Bucher, M.; Burigana, C.; Cardoso, J. F.; Catalano, A.; Challinor, A.; Chamballu, A.; Chiang, H. C.; Chiang, L. -Y.; Christensen, P. R.; Church, S.; Clements, D. L.; Colombi, S.; Colombo, L. P. L.; Couchot, F.; Coulais, A.; Crill, P.; Curto, A.; Cuttaia, F.; Danese, L.; Davies, R. D.; de Bernardis, P.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Delouis, J. -M.; Desert, F. -X.; Diego, J. M.; Dole, H.; Donzelli, S.; Dore, O.; Douspis, M.; Dupac, X.; Efstathiou, G.; Ensslin, T. A.; Eriksen, H. K.; Finelli, F.; Forni, O.; Frailis, M.; Franceschi, E.; Galeotta, S.; Gana, K.; Giard, M.; Girard, D.; Giraud-Heraud, Y.; Gonzalez-Nuevo, J.; Gorski, K. M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Hansen, F. K.; Hanson, D.; Harrison, D.; Henrot-Versille, S.; Hernandez-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hornstrup, Allan; Hovest, W.; Huffenberger, K. M.; Jaffe, A. H.; Jaffe, T. R.; Jones, W. C.; Juvela, M.; Keihanen, E.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knoche, J.; Knox, L.; Kunz, M.; Kurki-Suonio, H.; Lagache, G.; Lamarre, J. -M.; Lasenby, A.; Laureijs, R. J.; Lawrence, C. R.; Leonardi, R.; Leroy, C.; Lesgourgues, J.; Liguori, M.; Lilje, P. B.; Linden-Vørnle, Michael; Lopez-Caniego, M.; Lubin, P. M.; Macias-Perez, J. F.; Mandolesi, N.; Maris, M.; Marshall, D. J.; Martin, P. G.; Martinez-Gonzalez, E.; Masi, S.; Massardi, M.; Matarrese, S.; Matthai, F.; Mazzotta, P.; McGehee, P.; Melchiorri, A.; Mendes, L.; Mennella, A.; Migliaccio, M.; Miniussi, A.; Mitra, A.; Miville-Deschenes, M. A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Mottet, S.; Munshi, D.; Murphy, J. A.; Naselsky, P.; Nati, F.; Natoli, P.; Netterfield, C. B.; Nørgaard-Nielsen, Hans Ulrik; Noviello, F.; Novikov, D.; Novikov, I.; Osborne, S.; Oxborrow, Carol Anne; Paci, F.; Pagano, L.; Pajot, Fernand; Paoletti, D.; Patanchon, G.; Perdereau, O.; Perotto, L.; Perrotta, F.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Pietrobon, D.; Plaszczynski, S.; Pointecouteau, E.; Polenta, G.; Ponthieu, N.; Popa, L.; Poutanen, T.; Pratt, G. W.; Prezeau, G.; Prunet, S.; Puget, J. -L.; Rachen, J. P.; Racine, B.; Reinecke, M.; Remazeilles, M.; Renault, C.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Roudier, G.; Rusholme, B.; Sanselme, L.; Santos, D.; Sauve, A.; Savini, G.; Scott, D.; Shellard, E. P. S.; Spencer, L. D.; Starck, J. -L.; Stolyarov, V.; Stompor, R.; Sudiwala, R.; Sureau, F.; Sutton, D.; Suur-Uski, A. S.; Sygnet, J. -F.; Tauber, J. A.; Tavagnacco, D.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Tristram, M.; Tucci, M.; Umana, G.; Valenziano, L.; Valiviita, J.; Van Tent, B.; Vielva, P.; Villa, F.; Vittorio, N.; Wade, L. A.; Wandelt, B. D.; Yvon, D.; Zacchei, A.; Zonca, A.

In: Astronomy & Astrophysics, Vol. 571, A10, 2014, p. 23.

Research output: Contribution to journalJournal article – Annual report year: 2015Researchpeer-review

Harvard

Ade, PAR, Aghanim, N, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Battaner, E, Benabed, K, Benoit, A, Benoit-Levy, A, Bernard, J-P, Bersanelli, M, Bielewicz, P, Bobin, J, Bock, JJ, Bond, JR, Borrill, J, Bouchet, FR, Bridges, M, Bucher, M, Burigana, C, Cardoso, JF, Catalano, A, Challinor, A, Chamballu, A, Chiang, HC, Chiang, L-Y, Christensen, PR, Church, S, Clements, DL, Colombi, S, Colombo, LPL, Couchot, F, Coulais, A, Crill, P, Curto, A, Cuttaia, F, Danese, L, Davies, RD, de Bernardis, P, de Rosa, A, de Zotti, G, Delabrouille, J, Delouis, J-M, Desert, F-X, Diego, JM, Dole, H, Donzelli, S, Dore, O, Douspis, M, Dupac, X, Efstathiou, G, Ensslin, TA, Eriksen, HK, Finelli, F, Forni, O, Frailis, M, Franceschi, E, Galeotta, S, Gana, K, Giard, M, Girard, D, Giraud-Heraud, Y, Gonzalez-Nuevo, J, Gorski, KM, Gratton, S, Gregorio, A, Gruppuso, A, Hansen, FK, Hanson, D, Harrison, D, Henrot-Versille, S, Hernandez-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hivon, E, Hobson, M, Holmes, WA, Hornstrup, A, Hovest, W, Huffenberger, KM, Jaffe, AH, Jaffe, TR, Jones, WC, Juvela, M, Keihanen, E, Keskitalo, R, Kisner, TS, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lagache, G, Lamarre, J-M, Lasenby, A, Laureijs, RJ, Lawrence, CR, Leonardi, R, Leroy, C, Lesgourgues, J, Liguori, M, Lilje, PB, Linden-Vørnle, M, Lopez-Caniego, M, Lubin, PM, Macias-Perez, JF, Mandolesi, N, Maris, M, Marshall, DJ, Martin, PG, Martinez-Gonzalez, E, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, McGehee, P, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Miniussi, A, Mitra, A, Miville-Deschenes, MA, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Mottet, S, Munshi, D, Murphy, JA, Naselsky, P, Nati, F, Natoli, P, Netterfield, CB, Nørgaard-Nielsen, HU, Noviello, F, Novikov, D, Novikov, I, Osborne, S, Oxborrow, CA, Paci, F, Pagano, L, Pajot, F, Paoletti, D, Patanchon, G, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, GW, Prezeau, G, Prunet, S, Puget, J-L, Rachen, JP, Racine, B, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Riller, T, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rusholme, B, Sanselme, L, Santos, D, Sauve, A, Savini, G, Scott, D, Shellard, EPS, Spencer, LD, Starck, J-L, Stolyarov, V, Stompor, R, Sudiwala, R, Sureau, F, Sutton, D, Suur-Uski, AS, Sygnet, J-F, Tauber, JA, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Umana, G, Valenziano, L, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Vittorio, N, Wade, LA, Wandelt, BD, Yvon, D, Zacchei, A & Zonca, A 2014, 'HFI energetic particle effects: characterization, removal, and simulation', Astronomy & Astrophysics, vol. 571, A10, pp. 23. https://doi.org/10.1051/0004-6361/201321577

APA

Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., ... Zonca, A. (2014). HFI energetic particle effects: characterization, removal, and simulation. Astronomy & Astrophysics, 571, 23. [A10]. https://doi.org/10.1051/0004-6361/201321577

CBE

Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F, Aumont J, Baccigalupi C, Banday AJ, Barreiro RB, Battaner E, Benabed K, Benoit A, Benoit-Levy A, Bernard J-P, Bersanelli M, Bielewicz P, Bobin J, Bock JJ, Bond JR, Borrill J, Bouchet FR, Bridges M, Bucher M, Burigana C, Cardoso JF, Catalano A, Challinor A, Chamballu A, Chiang HC, Chiang L-Y, Christensen PR, Church S, Clements DL, Colombi S, Colombo LPL, Couchot F, Coulais A, Crill P, Curto A, Cuttaia F, Danese L, Davies RD, de Bernardis P, de Rosa A, de Zotti G, Delabrouille J, Delouis J-M, Desert F-X, Diego JM, Dole H, Donzelli S, Dore O, Douspis M, Dupac X, Efstathiou G, Ensslin TA, Eriksen HK, Finelli F, Forni O, Frailis M, Franceschi E, Galeotta S, Gana K, Giard M, Girard D, Giraud-Heraud Y, Gonzalez-Nuevo J, Gorski KM, Gratton S, Gregorio A, Gruppuso A, Hansen FK, Hanson D, Harrison D, Henrot-Versille S, Hernandez-Monteagudo C, Herranz D, Hildebrandt SR, Hivon E, Hobson M, Holmes WA, Hornstrup A, Hovest W, Huffenberger KM, Jaffe AH, Jaffe TR, Jones WC, Juvela M, Keihanen E, Keskitalo R, Kisner TS, Kneissl R, Knoche J, Knox L, Kunz M, Kurki-Suonio H, Lagache G, Lamarre J-M, Lasenby A, Laureijs RJ, Lawrence CR, Leonardi R, Leroy C, Lesgourgues J, Liguori M, Lilje PB, Linden-Vørnle M, Lopez-Caniego M, Lubin PM, Macias-Perez JF, Mandolesi N, Maris M, Marshall DJ, Martin PG, Martinez-Gonzalez E, Masi S, Massardi M, Matarrese S, Matthai F, Mazzotta P, McGehee P, Melchiorri A, Mendes L, Mennella A, Migliaccio M, Miniussi A, Mitra A, Miville-Deschenes MA, Moneti A, Montier L, Morgante G, Mortlock D, Mottet S, Munshi D, Murphy JA, Naselsky P, Nati F, Natoli P, Netterfield CB, Nørgaard-Nielsen HU, Noviello F, Novikov D, Novikov I, Osborne S, Oxborrow CA, Paci F, Pagano L, Pajot F, Paoletti D, Patanchon G, Perdereau O, Perotto L, Perrotta F, Piacentini F, Piat M, Pierpaoli E, Pietrobon D, Plaszczynski S, Pointecouteau E, Polenta G, Ponthieu N, Popa L, Poutanen T, Pratt GW, Prezeau G, Prunet S, Puget J-L, Rachen JP, Racine B, Reinecke M, Remazeilles M, Renault C, Ricciardi S, Riller T, Ristorcelli I, Rocha G, Rosset C, Roudier G, Rusholme B, Sanselme L, Santos D, Sauve A, Savini G, Scott D, Shellard EPS, Spencer LD, Starck J-L, Stolyarov V, Stompor R, Sudiwala R, Sureau F, Sutton D, Suur-Uski AS, Sygnet J-F, Tauber JA, Tavagnacco D, Terenzi L, Toffolatti L, Tomasi M, Tristram M, Tucci M, Umana G, Valenziano L, Valiviita J, Van Tent B, Vielva P, Villa F, Vittorio N, Wade LA, Wandelt BD, Yvon D, Zacchei A, Zonca A. 2014. HFI energetic particle effects: characterization, removal, and simulation. Astronomy & Astrophysics. 571:23. https://doi.org/10.1051/0004-6361/201321577

MLA

Vancouver

Ade PAR, Aghanim N, Armitage-Caplan C, Arnaud M, Ashdown M, Atrio-Barandela F et al. HFI energetic particle effects: characterization, removal, and simulation. Astronomy & Astrophysics. 2014;571:23. A10. https://doi.org/10.1051/0004-6361/201321577

Author

Ade, P. A. R. ; Aghanim, N. ; Armitage-Caplan, C. ; Arnaud, M. ; Ashdown, M. ; Atrio-Barandela, F. ; Aumont, J. ; Baccigalupi, C. ; Banday, A. J. ; Barreiro, R. B. ; Battaner, E. ; Benabed, K. ; Benoit, A. ; Benoit-Levy, A. ; Bernard, J. -P. ; Bersanelli, M. ; Bielewicz, P. ; Bobin, J. ; Bock, J. J. ; Bond, J. R. ; Borrill, J. ; Bouchet, F. R. ; Bridges, M. ; Bucher, M. ; Burigana, C. ; Cardoso, J. F. ; Catalano, A. ; Challinor, A. ; Chamballu, A. ; Chiang, H. C. ; Chiang, L. -Y. ; Christensen, P. R. ; Church, S. ; Clements, D. L. ; Colombi, S. ; Colombo, L. P. L. ; Couchot, F. ; Coulais, A. ; Crill, P. ; Curto, A. ; Cuttaia, F. ; Danese, L. ; Davies, R. D. ; de Bernardis, P. ; de Rosa, A. ; de Zotti, G. ; Delabrouille, J. ; Delouis, J. -M. ; Desert, F. -X. ; Diego, J. M. ; Dole, H. ; Donzelli, S. ; Dore, O. ; Douspis, M. ; Dupac, X. ; Efstathiou, G. ; Ensslin, T. A. ; Eriksen, H. K. ; Finelli, F. ; Forni, O. ; Frailis, M. ; Franceschi, E. ; Galeotta, S. ; Gana, K. ; Giard, M. ; Girard, D. ; Giraud-Heraud, Y. ; Gonzalez-Nuevo, J. ; Gorski, K. M. ; Gratton, S. ; Gregorio, A. ; Gruppuso, A. ; Hansen, F. K. ; Hanson, D. ; Harrison, D. ; Henrot-Versille, S. ; Hernandez-Monteagudo, C. ; Herranz, D. ; Hildebrandt, S. R. ; Hivon, E. ; Hobson, M. ; Holmes, W. A. ; Hornstrup, Allan ; Hovest, W. ; Huffenberger, K. M. ; Jaffe, A. H. ; Jaffe, T. R. ; Jones, W. C. ; Juvela, M. ; Keihanen, E. ; Keskitalo, R. ; Kisner, T. S. ; Kneissl, R. ; Knoche, J. ; Knox, L. ; Kunz, M. ; Kurki-Suonio, H. ; Lagache, G. ; Lamarre, J. -M. ; Lasenby, A. ; Laureijs, R. J. ; Lawrence, C. R. ; Leonardi, R. ; Leroy, C. ; Lesgourgues, J. ; Liguori, M. ; Lilje, P. B. ; Linden-Vørnle, Michael ; Lopez-Caniego, M. ; Lubin, P. M. ; Macias-Perez, J. F. ; Mandolesi, N. ; Maris, M. ; Marshall, D. J. ; Martin, P. G. ; Martinez-Gonzalez, E. ; Masi, S. ; Massardi, M. ; Matarrese, S. ; Matthai, F. ; Mazzotta, P. ; McGehee, P. ; Melchiorri, A. ; Mendes, L. ; Mennella, A. ; Migliaccio, M. ; Miniussi, A. ; Mitra, A. ; Miville-Deschenes, M. A. ; Moneti, A. ; Montier, L. ; Morgante, G. ; Mortlock, D. ; Mottet, S. ; Munshi, D. ; Murphy, J. A. ; Naselsky, P. ; Nati, F. ; Natoli, P. ; Netterfield, C. B. ; Nørgaard-Nielsen, Hans Ulrik ; Noviello, F. ; Novikov, D. ; Novikov, I. ; Osborne, S. ; Oxborrow, Carol Anne ; Paci, F. ; Pagano, L. ; Pajot, Fernand ; Paoletti, D. ; Patanchon, G. ; Perdereau, O. ; Perotto, L. ; Perrotta, F. ; Piacentini, F. ; Piat, M. ; Pierpaoli, E. ; Pietrobon, D. ; Plaszczynski, S. ; Pointecouteau, E. ; Polenta, G. ; Ponthieu, N. ; Popa, L. ; Poutanen, T. ; Pratt, G. W. ; Prezeau, G. ; Prunet, S. ; Puget, J. -L. ; Rachen, J. P. ; Racine, B. ; Reinecke, M. ; Remazeilles, M. ; Renault, C. ; Ricciardi, S. ; Riller, T. ; Ristorcelli, I. ; Rocha, G. ; Rosset, C. ; Roudier, G. ; Rusholme, B. ; Sanselme, L. ; Santos, D. ; Sauve, A. ; Savini, G. ; Scott, D. ; Shellard, E. P. S. ; Spencer, L. D. ; Starck, J. -L. ; Stolyarov, V. ; Stompor, R. ; Sudiwala, R. ; Sureau, F. ; Sutton, D. ; Suur-Uski, A. S. ; Sygnet, J. -F. ; Tauber, J. A. ; Tavagnacco, D. ; Terenzi, L. ; Toffolatti, L. ; Tomasi, M. ; Tristram, M. ; Tucci, M. ; Umana, G. ; Valenziano, L. ; Valiviita, J. ; Van Tent, B. ; Vielva, P. ; Villa, F. ; Vittorio, N. ; Wade, L. A. ; Wandelt, B. D. ; Yvon, D. ; Zacchei, A. ; Zonca, A. / HFI energetic particle effects: characterization, removal, and simulation. In: Astronomy & Astrophysics. 2014 ; Vol. 571. pp. 23.

Bibtex

@article{3b6e7cb3d6d14b75aad81edcb88af587,
title = "HFI energetic particle effects: characterization, removal, and simulation",
abstract = "We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1 K bolometer plate; and glitches in each detector time stream. The transient responses to detector glitch shapes are not simple single- pole exponential decays and fall into three families. The glitch shape for each family has been characterized empirically in flight data and these shapes have been used to remove glitches from the detector time streams. The spectrum of the count rate per unit energy is computed for each family and a correspondence is made to the location on the detector of the particle hit. Most of the detected glitches are from Galactic protons incident on the die frame supporting the micro- machined bolometric detectors. In the Planck orbit at L2, the particle flux is around 5 cm 2 s 1 and is dominated by protons incident on the spacecraft with energy > 39 MeV, at a rate of typically one event per second per detector. Di ff erent categories of glitches have di ff erent signatures in the time stream. Two of the glitch types have a low amplitude component that decays over nearly 1 s. This component produces excess noise if not properly removed from the time- ordered data. We have used a glitch detection and subtraction method based on the joint fit of population templates. The application of this novel glitch subtraction method removes excess noise from the time streams. Using realistic simulations, we find that this method does not introduce signal bias into the Planck data.",
keywords = "Cosmic background radiation, Cosmology: observations, Instrumentation: detectors, Space vehicles: instruments, Methods: data analysis, Astrophysics and Astronomy",
author = "Ade, {P. A. R.} and N. Aghanim and C. Armitage-Caplan and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and Banday, {A. J.} and Barreiro, {R. B.} and E. Battaner and K. Benabed and A. Benoit and A. Benoit-Levy and Bernard, {J. -P.} and M. Bersanelli and P. Bielewicz and J. Bobin and Bock, {J. J.} and Bond, {J. R.} and J. Borrill and Bouchet, {F. R.} and M. Bridges and M. Bucher and C. Burigana and Cardoso, {J. F.} and A. Catalano and A. Challinor and A. Chamballu and Chiang, {H. C.} and Chiang, {L. -Y.} and Christensen, {P. R.} and S. Church and Clements, {D. L.} and S. Colombi and Colombo, {L. P. L.} and F. Couchot and A. Coulais and P. Crill and A. Curto and F. Cuttaia and L. Danese and Davies, {R. D.} and {de Bernardis}, P. and {de Rosa}, A. and {de Zotti}, G. and J. Delabrouille and Delouis, {J. -M.} and Desert, {F. -X.} and Diego, {J. M.} and H. Dole and S. Donzelli and O. Dore and M. Douspis and X. Dupac and G. Efstathiou and Ensslin, {T. A.} and Eriksen, {H. K.} and F. Finelli and O. Forni and M. Frailis and E. Franceschi and S. Galeotta and K. Gana and M. Giard and D. Girard and Y. Giraud-Heraud and J. Gonzalez-Nuevo and Gorski, {K. M.} and S. Gratton and A. Gregorio and A. Gruppuso and Hansen, {F. K.} and D. Hanson and D. Harrison and S. Henrot-Versille and C. Hernandez-Monteagudo and D. Herranz and Hildebrandt, {S. R.} and E. Hivon and M. Hobson and Holmes, {W. A.} and Allan Hornstrup and W. Hovest and Huffenberger, {K. M.} and Jaffe, {A. H.} and Jaffe, {T. R.} and Jones, {W. C.} and M. Juvela and E. Keihanen and R. Keskitalo and Kisner, {T. S.} and R. Kneissl and J. Knoche and L. Knox and M. Kunz and H. Kurki-Suonio and G. Lagache and Lamarre, {J. -M.} and A. Lasenby and Laureijs, {R. J.} and Lawrence, {C. R.} and R. Leonardi and C. Leroy and J. Lesgourgues and M. Liguori and Lilje, {P. B.} and Michael Linden-V{\o}rnle and M. Lopez-Caniego and Lubin, {P. M.} and Macias-Perez, {J. F.} and N. Mandolesi and M. Maris and Marshall, {D. J.} and Martin, {P. G.} and E. Martinez-Gonzalez and S. Masi and M. Massardi and S. Matarrese and F. Matthai and P. Mazzotta and P. McGehee and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and A. Miniussi and A. Mitra and Miville-Deschenes, {M. A.} and A. Moneti and L. Montier and G. Morgante and D. Mortlock and S. Mottet and D. Munshi and Murphy, {J. A.} and P. Naselsky and F. Nati and P. Natoli and Netterfield, {C. B.} and N{\o}rgaard-Nielsen, {Hans Ulrik} and F. Noviello and D. Novikov and I. Novikov and S. Osborne and Oxborrow, {Carol Anne} and F. Paci and L. Pagano and Fernand Pajot and D. Paoletti and G. Patanchon and O. Perdereau and L. Perotto and F. Perrotta and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and T. Poutanen and Pratt, {G. W.} and G. Prezeau and S. Prunet and Puget, {J. -L.} and Rachen, {J. P.} and B. Racine and M. Reinecke and M. Remazeilles and C. Renault and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and B. Rusholme and L. Sanselme and D. Santos and A. Sauve and G. Savini and D. Scott and Shellard, {E. P. S.} and Spencer, {L. D.} and Starck, {J. -L.} and V. Stolyarov and R. Stompor and R. Sudiwala and F. Sureau and D. Sutton and Suur-Uski, {A. S.} and Sygnet, {J. -F.} and Tauber, {J. A.} and D. Tavagnacco and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and G. Umana and L. Valenziano and J. Valiviita and {Van Tent}, B. and P. Vielva and F. Villa and N. Vittorio and Wade, {L. A.} and Wandelt, {B. D.} and D. Yvon and A. Zacchei and A. Zonca",
year = "2014",
doi = "10.1051/0004-6361/201321577",
language = "English",
volume = "571",
pages = "23",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

RIS

TY - JOUR

T1 - HFI energetic particle effects: characterization, removal, and simulation

AU - Ade, P. A. R.

AU - Aghanim, N.

AU - Armitage-Caplan, C.

AU - Arnaud, M.

AU - Ashdown, M.

AU - Atrio-Barandela, F.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Battaner, E.

AU - Benabed, K.

AU - Benoit, A.

AU - Benoit-Levy, A.

AU - Bernard, J. -P.

AU - Bersanelli, M.

AU - Bielewicz, P.

AU - Bobin, J.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Bridges, M.

AU - Bucher, M.

AU - Burigana, C.

AU - Cardoso, J. F.

AU - Catalano, A.

AU - Challinor, A.

AU - Chamballu, A.

AU - Chiang, H. C.

AU - Chiang, L. -Y.

AU - Christensen, P. R.

AU - Church, S.

AU - Clements, D. L.

AU - Colombi, S.

AU - Colombo, L. P. L.

AU - Couchot, F.

AU - Coulais, A.

AU - Crill, P.

AU - Curto, A.

AU - Cuttaia, F.

AU - Danese, L.

AU - Davies, R. D.

AU - de Bernardis, P.

AU - de Rosa, A.

AU - de Zotti, G.

AU - Delabrouille, J.

AU - Delouis, J. -M.

AU - Desert, F. -X.

AU - Diego, J. M.

AU - Dole, H.

AU - Donzelli, S.

AU - Dore, O.

AU - Douspis, M.

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PY - 2014

Y1 - 2014

N2 - We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1 K bolometer plate; and glitches in each detector time stream. The transient responses to detector glitch shapes are not simple single- pole exponential decays and fall into three families. The glitch shape for each family has been characterized empirically in flight data and these shapes have been used to remove glitches from the detector time streams. The spectrum of the count rate per unit energy is computed for each family and a correspondence is made to the location on the detector of the particle hit. Most of the detected glitches are from Galactic protons incident on the die frame supporting the micro- machined bolometric detectors. In the Planck orbit at L2, the particle flux is around 5 cm 2 s 1 and is dominated by protons incident on the spacecraft with energy > 39 MeV, at a rate of typically one event per second per detector. Di ff erent categories of glitches have di ff erent signatures in the time stream. Two of the glitch types have a low amplitude component that decays over nearly 1 s. This component produces excess noise if not properly removed from the time- ordered data. We have used a glitch detection and subtraction method based on the joint fit of population templates. The application of this novel glitch subtraction method removes excess noise from the time streams. Using realistic simulations, we find that this method does not introduce signal bias into the Planck data.

AB - We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1 K bolometer plate; and glitches in each detector time stream. The transient responses to detector glitch shapes are not simple single- pole exponential decays and fall into three families. The glitch shape for each family has been characterized empirically in flight data and these shapes have been used to remove glitches from the detector time streams. The spectrum of the count rate per unit energy is computed for each family and a correspondence is made to the location on the detector of the particle hit. Most of the detected glitches are from Galactic protons incident on the die frame supporting the micro- machined bolometric detectors. In the Planck orbit at L2, the particle flux is around 5 cm 2 s 1 and is dominated by protons incident on the spacecraft with energy > 39 MeV, at a rate of typically one event per second per detector. Di ff erent categories of glitches have di ff erent signatures in the time stream. Two of the glitch types have a low amplitude component that decays over nearly 1 s. This component produces excess noise if not properly removed from the time- ordered data. We have used a glitch detection and subtraction method based on the joint fit of population templates. The application of this novel glitch subtraction method removes excess noise from the time streams. Using realistic simulations, we find that this method does not introduce signal bias into the Planck data.

KW - Cosmic background radiation

KW - Cosmology: observations

KW - Instrumentation: detectors

KW - Space vehicles: instruments

KW - Methods: data analysis

KW - Astrophysics and Astronomy

U2 - 10.1051/0004-6361/201321577

DO - 10.1051/0004-6361/201321577

M3 - Journal article

VL - 571

SP - 23

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A10

ER -